Titlebook: Interactions Between Physics and Dynamics of Solar System Bodies; Proceedings of the I E. Bois,P. Oberti,J. Henrard Conference proceedings

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The Trojan Asteroid Belt: Proper Elements, Stability, Chaos and Familiesed orbits, the stability of the proper elements-at least over 1 .- is within the following bounds: 0.001 . in semimajor axis, 0.0025 in eccentricity and sine of inclination. Half of the cases with degraded stability of the proper elements are found to be chaotic, with e-folding times between 16,000

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The Stability of the Planetary Three-Body Problem Influence of the Secular Resonancesspace for two planets in the neighbouring conditions of those of Jupiter and Saturn. The study of such a problem, which is more realistic than those based upon the K.A.M. theory, will lead us to give results of stability available in finite but very long time.

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Canonical Elements and Keplerian-Like Solutions for Intermediary Orbits of Satellites of an Oblate Ptificial Satellites of the Earth. In any case, the results are also applicable to problems dealing with orbital motion of other planetary satellites..The generality of this pattern leads to a . of solutions to the considered intermediaries: special choices of the Hamiltonian yield the corresponding

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Conference proceedings 1993 filled them with terror by describing the fate of the poor dinosaurs victims of a particularly nasty asteroid (or was it a comet?). You will be surprized to learn that Bretons did not exact a spectacular revenge for these offenses. On the contrary.

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